{"created":"2023-06-20T14:38:41.881814+00:00","id":5290,"links":{},"metadata":{"_buckets":{"deposit":"7bc97dd0-05e4-4283-954d-ac89e4462b91"},"_deposit":{"created_by":1,"id":"5290","owners":[1],"pid":{"revision_id":0,"type":"depid","value":"5290"},"status":"published"},"_oai":{"id":"oai:jaxa.repo.nii.ac.jp:00005290","sets":["1887:1891","9:789:956:959"]},"author_link":["25560","25559"],"item_5_biblio_info_10":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2009-02-27","bibliographicIssueDateType":"Issued"},"bibliographicPageEnd":"260","bibliographicPageStart":"256","bibliographicVolumeNumber":"JAXA-SP-08-014E","bibliographic_titles":[{"bibliographic_title":"宇宙航空研究開発機構特別資料"},{"bibliographic_title":"JAXA Special Publication: Astrophysics with All-Sky X-Ray observations: 3rd International MAXI Workshop","bibliographic_titleLang":"en"}]}]},"item_5_description_15":{"attribute_name":"会議概要（会議名, 開催地, 会期, 主催者等）（英）","attribute_value_mlt":[{"subitem_description":"Astrophysics with All-Sky X-Ray observations: 3rd International MAXI Workshop (RIKEN, 10-12 June 2008)","subitem_description_type":"Other"}]},"item_5_description_17":{"attribute_name":"抄録（英）","attribute_value_mlt":[{"subitem_description":"MAXI, Monitor of All-sky X-ray Image, is an X-ray observatory on the international space station. MAXI carries two kinds of slit scanning camera; gas slit camera (GSC) and solid-state slit camera (SSC). In the course of one station orbit, MAXI can scan almost the entire sky with a precision of 1.5 deg and with an X-ray energy range of 0.5 - 30 keV. Major purpose of MAXI is monitor of known X-ray sources and detection of new serendipitous sources such as X-ray nova whereas diffuse X-ray emission in our galaxy is also an important target especially for SSC. The good energy resolving power of SSC enables us, for the first time, to map the entire sky with various line emission from O to Fe. Based on the previous observational data, we simulate MAXI data both for SSC and GSC. Large-scale structures in our galaxy such as supernova remnants, radio loop, superbubbles are possible targets for SSC. The Galactic ridge X-ray emission is important target both for GSC and SSC.","subitem_description_type":"Other"}]},"item_5_description_32":{"attribute_name":"資料番号","attribute_value_mlt":[{"subitem_description":"資料番号: AA0064306051","subitem_description_type":"Other"}]},"item_5_description_33":{"attribute_name":"レポート番号","attribute_value_mlt":[{"subitem_description":"レポート番号: JAXA-SP-08-014E","subitem_description_type":"Other"}]},"item_5_publisher_8":{"attribute_name":"出版者","attribute_value_mlt":[{"subitem_publisher":"宇宙航空研究開発機構"}]},"item_5_publisher_9":{"attribute_name":"出版者（英）","attribute_value_mlt":[{"subitem_publisher":"Japan Aerospace Exploration Agency (JAXA)"}]},"item_5_source_id_21":{"attribute_name":"ISSN","attribute_value_mlt":[{"subitem_source_identifier":"1349-113X","subitem_source_identifier_type":"ISSN"}]},"item_5_source_id_24":{"attribute_name":"書誌レコードID","attribute_value_mlt":[{"subitem_source_identifier":"AA11984031","subitem_source_identifier_type":"NCID"}]},"item_5_text_6":{"attribute_name":"著者所属","attribute_value_mlt":[{"subitem_text_value":"大阪大学理学研究科宇宙地球学専攻"}]},"item_5_text_7":{"attribute_name":"著者所属（英）","attribute_value_mlt":[{"subitem_text_language":"en","subitem_text_value":"Department of Earth & Space Science, Graduate School of Science, Osaka University"},{"subitem_text_language":"en","subitem_text_value":"MAXI Team"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"宮田, 恵美"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Miyata, Emi","creatorNameLang":"en"}],"nameIdentifiers":[{}]}]},"item_files":{"attribute_name":"ファイル情報","attribute_type":"file","attribute_value_mlt":[{"accessrole":"open_date","date":[{"dateType":"Available","dateValue":"2020-01-16"}],"displaytype":"detail","filename":"64306051.pdf","filesize":[{"value":"507.3 kB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"64306051.pdf","url":"https://jaxa.repo.nii.ac.jp/record/5290/files/64306051.pdf"},"version_id":"14341ba1-b65a-4bdf-b908-c4af90e20082"}]},"item_keyword":{"attribute_name":"キーワード","attribute_value_mlt":[{"subitem_subject":"X-ray - all-sky survey - diffuse source - all-sky line map","subitem_subject_language":"en","subitem_subject_scheme":"Other"}]},"item_language":{"attribute_name":"言語","attribute_value_mlt":[{"subitem_language":"eng"}]},"item_resource_type":{"attribute_name":"資源タイプ","attribute_value_mlt":[{"resourcetype":"conference paper","resourceuri":"http://purl.org/coar/resource_type/c_5794"}]},"item_title":"Diffuse source mapping with MAXI","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"Diffuse source mapping with MAXI","subitem_title_language":"en"}]},"item_type_id":"5","owner":"1","path":["959","1891"],"pubdate":{"attribute_name":"公開日","attribute_value":"2015-03-26"},"publish_date":"2015-03-26","publish_status":"0","recid":"5290","relation_version_is_last":true,"title":["Diffuse source mapping with MAXI"],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2023-06-21T08:18:32.124392+00:00"}